output
20022026
most citedGW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

9.8k citations

Showing 2003 · astro-phShow all

11 papers · 2 filters

astro-ph2003

Automated Determination of Stellar Population Parameters in Galaxies Using Active Instance-based Learning

Thamar Solorio, Olac Fuentes, Roberto Terlevich +2

In this work we focus on the determination of the relative distributions of young, intermediate-age and old populations of stars in galaxies. Starting from a grid of theoretical po…

astro-ph2003

Central DM density cuspiness in LSB's: a stellar kinematics approach

A. Pizzella, E. M. Corsini, F. Bertola +4

We present preliminary results from spectroscopic observations of a sample of 11 low surface brightness galaxies (LSB). We measured the stellar and gaseous kinematics along their m…

astro-ph2003

The sigma_c-V_c correlation in high and low surface brightness galaxies

A. Pizzella, E. Dalla Bonta', E. M. Corsini +2

We investigate the relation between the central velocity dispersion, sigma_0, and the circular velocity, V_c, in galaxies. In addition to previously available data, we consider an…

astro-ph2003

Spectroscopy, Photometry and Micro-arcsec Astrometry of Binaries with the GAIA Space Mission and with the RAVE Experiment

Tomaz Zwitter, Ulisse Munari

GAIA astrometric mission of ESA will be very efficient in discovering binary and multiple stars with any orbital period, from minutes to millions of years. Main parameters of the r…

astro-ph2003

Variable stars as tracers of stellar populations in Local Group galaxies: Leo I and NGC 6822

L. Baldacci, F. Matonti, L. Rizzi +5

Results are presented of a study of the variable star populations in the dwarf spheroidal galaxy Leo I and in the dwarf irregular galaxy NGC 6822, based on time series photometry o…

astro-ph2003

The Red Giant Branch Bump

M. Riello, G. Piotto, A. Recio-Blanco +2

We present a comparison between theoretical models and the observed magnitude difference between the horizontal branch and the red giant branch bump for a sample of 53 clusters. We…